概括
大质量恒星中的 (22) Ne ((alpha,n) ((23) Mg反应产生了铁-59和-60.等s过程元素. 这些元素的马射线应该可以从大多数II型超新星中检测到.
科学领域:
- 核天体物理学 核天体物理学
- 恒星进化中的恒星演变
- 超新星的核合成
背景情况:
- 在大质量恒星中燃烧的对于元素生产至关重要.
- s过程 (缓慢的中子捕获) 是一个关键的核合成途径.
- 了解超新星前的状况,可以为超新星观测提供信息.
研究的目的:
- 为了计算超新星前恒星的燃烧外中的核丰度.
- 通过中子捕获反应研究特定同位素的产生.
- 为了预测超新星残余的玛射线辐射的可检测性.
主要方法:
- 在恒星内部建模核丰度.
- 模拟通过 (22) Ne ((alpha,n) ((23) Mg反应的中子产生.
- 通过超新星冲击波评估合成的同位素的生存.
主要成果:
- 对于恒星> 20 太阳质量, (22) Ne ((alpha,n) ((23) Mg反应产生足够的中子用于s过程核合成.
- 合成了铁-59 (半衰期45天) 和-60 (半衰期5.3年).
- 预计这些同位素能够在超新星冲击中存活下来.
结论:
- 来自铁-59和-60衰变的马射线应该可以从大多数银河系II型超新星中检测到.
- 这些特定的马射线不太可能从超新星1987A中观察到,因为它的距离和低金属度.
相关概念视频
Types of Radioactivity
The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Emission Spectra
When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
Radioactivity and Nuclear Equations
Nuclear chemistry is the study of reactions that involve changes in nuclear structure. The nucleus of an atom is composed of protons and, except for hydrogen, neutrons. The number of protons in the nucleus is called the atomic number (Z) of the element, and the sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are isotopes of the same element.
A nuclide of an element has a specific number of protons and...
A nuclide of an element has a specific number of protons and...
Nuclear Stability
Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively charged protons together in the...
To hold positively charged protons together in the...
Nuclear Transmutation
Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed protons being...
Atomic Nuclei: Types of Nuclear Relaxation
Nuclear relaxation restores the equilibrium population imbalance and can occur via spin–lattice or spin–spin mechanisms, which are first-order exponential decay processes.
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers energy to a nearby...
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers energy to a nearby...


